Piercing of a solitonic boson star by a black hole
Autor(a) principal: | |
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Data de Publicação: | 2023 |
Outros Autores: | , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
Texto Completo: | http://hdl.handle.net/10773/39696 |
Resumo: | Recently, the piercing of a mini boson star by a black hole was studied, with tidal capture and the discovery of a “gravitational atom” being reported [Cardoso et al., Phys. Rev. D 106, 044030 (2022).]. Building on this research, we extend the study by including a hexic solitonic potential and explore the piercing of a solitonic boson star by a black hole. Notably, the solitonic boson star can reach higher compactness, which one might expect could alter the dynamics in this context. Our findings suggest that even when the black hole’s size approaches the test particle limit, the solitonic boson star is easily captured by the black hole due to an extreme tidal capture process. Regardless of the black hole initial mass and velocity, our results indicate that over 85% of the boson star material is accreted. Thus, the self-interaction does not alter the qualitative behavior of the system. |
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Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
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Piercing of a solitonic boson star by a black holeRecently, the piercing of a mini boson star by a black hole was studied, with tidal capture and the discovery of a “gravitational atom” being reported [Cardoso et al., Phys. Rev. D 106, 044030 (2022).]. Building on this research, we extend the study by including a hexic solitonic potential and explore the piercing of a solitonic boson star by a black hole. Notably, the solitonic boson star can reach higher compactness, which one might expect could alter the dynamics in this context. Our findings suggest that even when the black hole’s size approaches the test particle limit, the solitonic boson star is easily captured by the black hole due to an extreme tidal capture process. Regardless of the black hole initial mass and velocity, our results indicate that over 85% of the boson star material is accreted. Thus, the self-interaction does not alter the qualitative behavior of the system.American Physical Society2023-11-15T15:45:21Z2023-07-05T00:00:00Z2023-07-05info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10773/39696eng1550-799810.1103/PhysRevD.108.084051Zhong, ZhenCardoso, VitorIkeda, TaishiZilhão, Miguelinfo:eu-repo/semantics/openAccessreponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãoinstacron:RCAAP2024-02-22T12:17:40Zoai:ria.ua.pt:10773/39696Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-20T03:09:51.317967Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãofalse |
dc.title.none.fl_str_mv |
Piercing of a solitonic boson star by a black hole |
title |
Piercing of a solitonic boson star by a black hole |
spellingShingle |
Piercing of a solitonic boson star by a black hole Zhong, Zhen |
title_short |
Piercing of a solitonic boson star by a black hole |
title_full |
Piercing of a solitonic boson star by a black hole |
title_fullStr |
Piercing of a solitonic boson star by a black hole |
title_full_unstemmed |
Piercing of a solitonic boson star by a black hole |
title_sort |
Piercing of a solitonic boson star by a black hole |
author |
Zhong, Zhen |
author_facet |
Zhong, Zhen Cardoso, Vitor Ikeda, Taishi Zilhão, Miguel |
author_role |
author |
author2 |
Cardoso, Vitor Ikeda, Taishi Zilhão, Miguel |
author2_role |
author author author |
dc.contributor.author.fl_str_mv |
Zhong, Zhen Cardoso, Vitor Ikeda, Taishi Zilhão, Miguel |
description |
Recently, the piercing of a mini boson star by a black hole was studied, with tidal capture and the discovery of a “gravitational atom” being reported [Cardoso et al., Phys. Rev. D 106, 044030 (2022).]. Building on this research, we extend the study by including a hexic solitonic potential and explore the piercing of a solitonic boson star by a black hole. Notably, the solitonic boson star can reach higher compactness, which one might expect could alter the dynamics in this context. Our findings suggest that even when the black hole’s size approaches the test particle limit, the solitonic boson star is easily captured by the black hole due to an extreme tidal capture process. Regardless of the black hole initial mass and velocity, our results indicate that over 85% of the boson star material is accreted. Thus, the self-interaction does not alter the qualitative behavior of the system. |
publishDate |
2023 |
dc.date.none.fl_str_mv |
2023-11-15T15:45:21Z 2023-07-05T00:00:00Z 2023-07-05 |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://hdl.handle.net/10773/39696 |
url |
http://hdl.handle.net/10773/39696 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
1550-7998 10.1103/PhysRevD.108.084051 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
dc.publisher.none.fl_str_mv |
American Physical Society |
publisher.none.fl_str_mv |
American Physical Society |
dc.source.none.fl_str_mv |
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instname_str |
Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação |
instacron_str |
RCAAP |
institution |
RCAAP |
reponame_str |
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
collection |
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
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Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação |
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1799137748815183872 |